Star formation around RCW 120, the perfect bubble

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Free access article

Issue		A&A Volume 496, Number 1, March II 2009


Page(s)		177 - 190
Section		Interstellar and circumstellar matter
DOI		http://dx.doi.org/10.1051/0004-6361/200811337
Published online		30 January 2009

A&A 496, 177-190 (2009)
DOI: 10.1051/0004-6361/200811337

Star formation around RCW 120, the perfect bubble

L. Deharveng¹, A. Zavagno¹, F. Schuller², J. Caplan¹, M. Pomarès¹, and C. De Breuck³

¹ Laboratoire d'Astrophysique de Marseille (UMR 6110 CNRS & Université de Provence), 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, France
e-mail: Lise.Deharveng@oamp.fr
² Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
³ European Southern Observatory, Karl-Schwarschild Strasse, 85748 Garching bei München, Germany

Received 12 November 2008 / Accepted 7 January 2009

Abstract
Context. This study deals with the star formation triggered by H II regions.
Aims. We wish to take advantage of the very simple morphology of RCW 120 – a perfect bubble – to understand the mechanisms triggering star formation around an H II region and to establish what kind of stars are formed there.
Methods. We present 870 $\mu$ m observations of RCW 120, obtained with the APEX-LABOCA camera. These show the distribution of cold dust, and thus of neutral material. We use Spitzer-MIPS observations at 24 $\mu$ m and 70 $\mu$ m to detect the young stellar objects present in this region and to estimate their evolutionary stages.
Results. A layer of dense neutral material surrounds the entire H II region, having been swept up during the region's expansion. This layer has a mass greater than $2000~M_{\odot}$ and is fragmented, with massive fragments elongated along the ionization front (IF). We measured the 24 $\mu$ m flux of 138 sources. Of these, 39 are Class I or flat-spectrum young stellar objects (YSOs) observed in the direction of the collected layer. We show that several triggering mechanisms are acting simultaneously in the swept-up shell, where they form a second generation of stars. No massive YSOs are detected. However, a massive, compact 870 $\mu$ m core lies adjacent to the IF. A 70 $\mu$ m source with no 24 $\mu$ m counterpart is detected at the same position. This source is a likely candidate for a Class 0 YSO. Also at 24 $\mu$ m, we detect a chain of about ten regularly spaced Class I or flat spectrum sources, parallel to the IF, in the direction of the most massive fragment. We suggest that the formation of these YSOs is the result of Jeans gravitational instabilities in the collected layer. Finally, the 870 $\mu$ m emission, the 24 $\mu$ m emission, and the H $\alpha$ emission show the existence of an extended and partially ionized photodissociation region around RCW 120. This demonstrates the long-distance influence of the H II region upon its surrounding medium.

Key words: stars: formation -- stars: early-type -- ISM: H II regions -- ISM: individual objects: RCW 120

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